Quantum Leaps in the Vicinity of One-Loop Gravity Black Holes

Abstract

Consider a non-stationary extension of black hole solutions to the quantum-extended (one-loop GR) system of Einstein–Maxwell equations with a complex scalar field. Important representatives of these solutions are non-stationary rotating black holes located inside the active galactic nuclei. Computing the local energy density of a freely falling observer one finds, upon appropriate boundary conditions, the trans-Planckian leap of the local energy density near the event horizons. Thus, one locates a “Firewall”, which, on one hand, serves as a source of fluxes of ultra-high-energy cosmic rays out of the active galactic nuclei, and, on the other hand, is originally designed to resolve the Hawking paradox in black hole physics.